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Weblio 辞書 > 英和辞典・和英辞典 > λに関連した共起表現

「λ」の共起表現一覧(1語右で並び替え)

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Introducing an undetermined multiplier λ, a Lagrangian is constructed as
and for λ an infinite limit ordinal,
the process (a, λ).P can perform an action a at rate λ and continu
If the (m+1)th order of λ and (m)th order of (λ + Δλ) lie at the same angl
ty, compact sets) K and L with probabilities 1 − λ and λ respectively, then Vitale's random Brunn-M
the following property: there exists a worldline λ and an event p such that all events along λ are
del with the critical point of j being κ, j(κ) ≥ λ, and V(λ) is a subset of j(M).
onformations, which are described by the symbols λ and δ.
he two groups are proportional with hazard ratio λ and d1 and d2 are the probabilities that a subje
ate, which can be resolved into two enantiomers ( Λ and Δ) by the formation of the d-α-bromocamphor-
In such a case we need a better first guess at λ, and that may not be easy to get; the alternativ
Lambda Andromedae ( λ And, λ Andromedae) is a binary star in the const
Lambda Aquilae ( λ Aql, λ Aquilae) is a star in the constellation A
Lambda Aquarii ( λ Aqr, λ Aquarii) is a star in the constellation A
where λ are mean longitudes of the moons.
The Lyapunov exponents, λ are approximately 0.1981, 0, −0.6581 and the Kap
rmula may fail to converge; this will occur when λ as computed by the equation above is greater tha
Lambda Aurigae ( λ Aur, λ Aurigae) is a binary star in the constell
Its companion, λ Aurigae B, is 29 arcseconds away and has an appa
o has two optical companions, the 12th magnitude λ Aurigae C at 42 arcseconds and the magnitude +8.
The primary component, λ Aurigae A, is a yellow G-type subgiant with an a
In particle physics, lambda ( Λ) baryons are baryons containing an up quark, a d
any two varieties occur together in exactly λ blocks;
of the particle p was related to its wavelength λ by what is now known as the de Broglie relation
nt of the group of quaternionic automorphisms of Λ by the group ±1 of scalars.
yle of obtaining the normal form of terms in the λ calculus by appealing to their denotational sema
oncept of "effective calculability" based on his λ calculus and by Alan Turing in the same year wit
λ Canis Majoris is a blue-white B-type main sequen
β Cassiopeiae, κ Cassiopeiae, η Cassiopeiae and λ Cassiopeiae.
Lambda Centauri ( λ Cen, λ Centauri) is a star in the constellation
λ Centauri is a blue-white B-type giant with an ap
This star, along with α Cet (Menkar), λ Cet (Menkar), γ Cet (Kaffaljidhma), μ Cet, ξ1 Ce
is star, along with γ Cet (Kaffaljidhma), δ Cet, λ Cet (Menkar), μ Cet, ξ1 Cet and ξ2 Cet were Al K
Cet as Al Kaff al Jidhmah IV (exclude α Cet and λ Cet)
Lambda Canis Majoris ( λ CMa, λ Canis Majoris) is a star in the constella
Aksys Games released Λ Core Plus for the US market on April 7, 2009 for
The apparent magnitude of λ Crucis is 4.6, but it is not stable.
λ Crucis is located at 360 light-years from the Su
Lambda Crucis ( λ Crucis / λ Cru) is a star in the constellation C
where λ denotes Lebesgue measure and ρ is the backward s
B. (1982), "Nucleotide sequence of bacteriophage λ DNA", Journal of Molecular Biology 162 (4): 729-
For example, a λ DNA-HindIII Digest: a common lambda DNA ladder t
tar association consisting this star, along with λ Eri, ψ Eri and τ Ori
y assigning the zero mass particles a small mass λ, evaluating the corresponding expression and the
Lambda Geminorum ( λ Gem, λ Geminorum) is a Class A3, fourth-magnitud
crystals, there is a minimum possible wavelength λ, given by twice the equilibrium separation betwe
With β, δ, θ. ι, and λ Gru, it belonged to Piscis Austrinus in traditio
of the (Southern) Fish: it, with α, δ, θ. ι, and λ Gru, belonged to Piscis Austrinus in traditional
node i carries, Ai,j is the adjacency matrix and λ happens to be the principal eigenvalue (although
where Λ has a finite value that represents the fastest d
eigenvector of Th with respect to the eigenvalue λ, i.e.
ss fin of the last record of the output list (or Λ if that list is still empty).
bedding j:(Vκ, ∈, P) → (Vλ, ∈, P) for some κ and λ in S.
behaviour (measured using the Lyapunov exponent λ) in the a−b plane for a given periodic sequence
attP and attB of λ integrase, see lambda phage).
If Λ is a harmonious set and F is a finite set then t
A set Λ is harmonious if every weak character may be app
If λ is any ordinal, κ is λ-supercompact means that t
Where D00 is the beam waist size, and λ is the wavelength.
successor operation S; in precise terms, we say λ is a limit ordinal if and only if λ > 0 and for
The value of the cosmological constant, Λ, is ~2 x 10−35s−2.
where λ is the wavelength of the spectral peak of intere
where λ is the Marquardt parameter and I is an identity
where λ is the wavelength, f is the frequency, and c is
Sometimes, a cosmological constant Λ is included in the Lagrangian so that the new ac
If λ is any ordinal, κ is λ-strong means that κ is a
e a is the period of the diffraction grating and λ is the wavelength of the light incident on the g
ength (distance from pinhole to image plane) and λ is the wavelength of light.
he radiator (or the diametre of the antenna) and λ is the wavelength of the radio wave.
into a transitive class M that includes Vλ where λ is the first fixed point above the critical poin
ope as , where d is the resolvable feature size, λ is the wavelength of light, n is the index of re
er model M with critical point κ and λM⊆M, where λ is the supremum of jnκ for positive integers n.
λ is the mean free path
Λ is a set of formal languages;
where λ is the signal's wavelength.
Phoenician letter gave rise to the Greek Lambda ( Λ), Latin L, and Cyrillic El (Л).
Since λ lies in p's past, the Turing machine can signal
Lambda Lyrae ( λ Lyr) is a 5th magnitude star in the constellatio
Color the point (a,b) according to the value of λ obtained.
Because only certain wavelengths ( λ) of light are absorbed - those matching exactly
A strong character is a restriction to Λ of a continuous homomorphism from G to T, that i
Lambda Ophiuchi ( λ Oph, λ Ophiuchi) is a binary star system in the
It is denoted with λ or sometimes Λ or ε.
λ Ori X-1 has visual designation HDE 245059.
The Orion X-ray source, λ Ori X-1, is not in any Uhuru catalog.
λ Ori X-1 is actually a discovery with the Einstei
λ Ori X-1 is spectral type K1, rotating at ~25 km/
λ Ori is one of the youngest stars of the λ Ori as
Lambda Orionis ( λ Ori, λ Orionis) is a star in the constellation O
ena), but was somehow also mistakenly applied to λ Orionis and the name stuck.
ion of either a lytic or lysogenic life cycle in λ phage - with high concentrations of cIII promoti
S → λ provided S does not appear on the right side of
where λ represents the gaugino field (a spinor) and Λ is
λ Sco and υ Sco, two stars at the end of the scorp
Lambda Serpentis ( λ Ser, λ Serpentis) is a star in the constellation
Lambda Sagittarii ( λ Sgr, λ Sagittarii) is a star within the constell
(named for W. Hugh Woodin) is a cardinal number λ such that for all functions
Along with λ Tau, it was one of the first stars on which rota
Lambda Telescopii ( λ Tel, λ Telescopii) is a star in the constellatio
distributed random variable hain with parameter λ, that is, with probability density function
with n0 the refractive index of the solvent, λ the wavelength of the light source, dn/dc the re
Here Nx is the number of x atoms per volume, λ the electron escape depth, θ the analyzer angle,
th s the shear distance, df the fringe distance, λ the wavelength and γ the angular deviation of th
with a Poisson distribution with expected value λ, then its nth moment is
inal number κ is called η-extendible if for some λ there is a nontrivial elementary embedding j of
The World Is a Thorn (also stylized The World Is Λ Thorn) is Demon Hunter's fifth studio album, whi
rent precision electroweak measurements restrict Λ to more than a few TeV.
This causes the wavelength λ to decrease, which means that the signal then tr
he small quantum cohomology with coefficients in Λ to be
Lambda Ursae Majoris ( λ UMa, λ Ursae Majoris) is a star in the constella
ved into enantiomers that are described as Δ and Λ. Usually the resolution entails use of tartrate s
Lambda Velorum ( λ Vel or λ Velorum) is a star in the constellation
gen "fuel" much faster than do smaller stars and λ Velorum is estimated to be only some 27 million
Lambda Virginis ( λ Vir, λ Virginis) is a binary star in the constel
tements has cardinality below a certain cardinal λ; we may then refer to λ-compactness.
Compton recoil with momentum proportional to h / λ, where h is Planck's constant.
                                                                                                   


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